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arXiv 2212.04413physics.atom-phhep-ph
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利用射频原子跃迁光谱学寻找超轻暗物质

Search for ultralight dark matter with spectroscopy of radio-frequency atomic transitions

Xue Zhang, Abhishek Banerjee, Mahapan Leyser, Gilad Perez, Stephan Schiller, Dmitry Budker, Dionysios Antypas

AI总结:

通过对比石英振荡器与铷、镝原子跃迁频率,搜寻标量与赝标量超轻玻色子暗物质,对特定质量范围内的暗物质与标准模型场的线性和二次相互作用给出了超越以往直接搜索及天体物理观测的约束。

摘要:

通过将石英振荡器的频率与$^{87}$Rb的超精细结构跃迁以及$^{164}$Dy的电子跃迁频率进行比较,我们搜寻了标量和赝标量超轻玻色子暗物质(UBDM)的效应。对于处于$1\times10^{-17}-8.3\times10^{-13}$ eV范围内的UBDM粒子质量,我们约束了标量UBDM场与标准模型(SM)场之间的线性相互作用;对于$5\times10^{-18}-4.1\times10^{-13}$ eV范围内的质量,约束了赝标量UBDM场与SM场之间的二次相互作用。在各自范围的相应区域内,我们对线性相互作用的约束显著改进了先前对原子参数振荡的直接搜索结果,而对二次相互作用的约束则超越了此类直接搜索以及天体物理观测所设定的限制。

英文摘要:

The effects of scalar and pseudoscalar ultralight bosonic dark matter (UBDM) were searched for by comparing the frequency of a quartz oscillator to that of a hyperfine-structure transition in $^{87}$Rb, and an electronic transition in $^{164}$Dy. We constrain linear interactions between a scalar UBDM field and Standard-Model (SM) fields for an underlying UBDM particle mass in the range $1\times10^{-17}-8.3\times10^{-13} $ eV and quadratic interactions between a pseudoscalar UBDM field and SM fields in the range $5\times10^{-18}- 4.1\times10^{-13} $ eV. Within regions of the respective ranges, our constraints on linear interactions significantly improve on results from previous, direct searches for oscillations in atomic parameters, while constraints on quadratic interactions surpass limits imposed by such direct searches as well as by astrophysical observations.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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